Waves and Optics: cram pack

Formula sheets, the key method steps for every topic and 4 practice problems, with full solutions at the back.

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1Formulas and methods

Springs & pendulums

Mass on a spring
T = 2π·√(m/k)
Pendulum
T = 2π·√(L/g)
Angular frequency
ω = √(k/m) = 2π/T
Maximum speed and acceleration
vmax = A·ω, amax = A·ω²
Energy
E = ½·k·A²

Waves, sound & optics

Wave speed
v = fλ, T = 1/f
String
v = √(T/μ), μ = m/L
Sound level
β = 10·log10(I/I0), I0 = 10⁻¹² W/m²
Point source
I = P/(4πr²)
Standing waves
string or open pipe fn = n·v/(2L); closed pipe fn = n·v/(4L), n odd
Doppler effect
f′ = f·(v ± vo)/(v ∓ vs)
Refractive index
n = c/v, λ = λ0/n
Snell’s law
n1sin θ1 = n2sin θ2
Critical angle
sin θc = n2/n1
Optical fibre
NA = sin θa = √(n1² − n2²)
Lenses and mirrors
1/f = 1/do + 1/di, m = −di/do, mirror f = R/2
Double slit
d·sin θ = mλ, ym = mλL/d
Grating
d = 1/N, d·sin θ = mλ, mmax ≤ d/λ
Single slit
a·sin θ = mλ (dark), w = 2λL/a

Method

  1. Identify the kind of problem: wave speed, sound level, standing wave, Doppler, refraction, lens or mirror, or interference.
  2. Write the relation first: v = fλ, β = 10·log(I/I₀), fₙ = n·v/(2L) or n·v/(4L), f′ = f(v ± vo)/(v ∓ vs), n₁sin θ₁ = n₂sin θ₂, 1/f = 1/d₀ + 1/dᵢ, d·sin θ = mλ.
  3. Convert units: nm, mm and cm to m, and check whether angles are measured from the normal.
  4. Check signs and plausibility: a virtual image has dᵢ < 0, an approaching source sounds higher, a closed pipe has only odd harmonics.

2Practice problems

1.Springs & pendulumsMedium
L = 0.5 mT = 1.33 s

An astronaut on another planet finds that a simple pendulum 0.5 m long has a period of 1.33 s for small swings. Find the gravitational acceleration g on that planet.

L = 0.5 mT = 1.33 s
g = m/s²
2.Springs & pendulumsHard
1.5 kgk = 140 N/mA = 9 cm

A 1.5 kg mass on a spring with k = 140 N/m is pulled 9 cm from equilibrium and released. Find its maximum speed vmax.

m = 1.5 kgk = 140 N/mA = 9 cm
vmax = m/s
3.Waves, sound & opticsMedium
L = 0.6 mn = 2

A string fixed at both ends is 0.6 m long; waves travel on it at 100 m/s. Find the frequency f2 of its harmonic number 2.

v = 100 m/sn = 2L = 0.6 m
f2 = Hz
4.Waves, sound & opticsHard
θn1​ = 1.5n2​ = 1.42n0​ = 1.00

An optical fibre has a core with n₁ = 1.5 and a cladding with n₂ = 1.42. Find its numerical aperture NA.

n1 = 1.5n2 = 1.42
NA =

3Solutions

1.Springs & pendulums

Answer: g = 11.16 m/s²

Simple harmonic motion: a mass m on a spring of stiffness k oscillates with angular frequency ω = √(k/m) and period T = 2π/ω = 2π·√(m/k). A simple pendulum of length L has T = 2π·√(L/g). With amplitude A, the largest speed is A·ω, the largest acceleration A·ω² and the energy ½·k·A².

Solve for g

g = 4π²·L/T² = 4π²·0.5/1.33² = 11.16 m/s²

Answer

g = 11.16 m/s²
2.Springs & pendulums

Answer: vmax = 0.8695 m/s

Simple harmonic motion: a mass m on a spring of stiffness k oscillates with angular frequency ω = √(k/m) and period T = 2π/ω = 2π·√(m/k). A simple pendulum of length L has T = 2π·√(L/g). With amplitude A, the largest speed is A·ω, the largest acceleration A·ω² and the energy ½·k·A².

Angular frequency

ω = √(140/1.5) = 9.661 rad/s

Maximum speed

vmax = A·ω = 0.09·9.661 = 0.8695 m/s

Answer

vmax = 0.8695 m/s
3.Waves, sound & optics

Answer: f2 = 166.7 Hz

Standing waves and the Doppler effect: a string fixed at both ends, or a pipe open at both ends, fits whole half-wavelengths: L = nλ/2, fn = n·v/(2L), n = 1, 2, 3, … A pipe closed at one end has a node at the closed end and an antinode at the open end: L = nλ/4 with odd n only, fn = n·v/(4L). When source or observer move along the line between them, f′ = f·(v ± vo)/(v ∓ vs): use the upper signs for motion towards each other. Two waves of nearly equal frequency beat at |f₁ − f₂|.

Wavelength of this mode

λ = 2L/n = 2·0.6/2 = 0.6 m

Frequency

f = v/λ = 100/0.6 = 166.7 Hz

Answer

f2 = 166.7 Hz
4.Waves, sound & optics

Answer: NA = 0.4833

Geometric optics: at a boundary, n₁·sin θ₁ = n₂·sin θ₂ (Snell's law), with angles measured from the normal and n = c/v. Going into a slower medium the ray bends towards the normal. From a denser medium (n₁ > n₂) beyond the critical angle θc = arcsin(n₂/n₁) all light is reflected: total internal reflection. Thin lenses and spherical mirrors obey 1/f = 1/do + 1/di with the magnification m = −di/do. Sign convention: f > 0 for a converging lens and a concave mirror (f = R/2), f < 0 for a diverging lens and a convex mirror; di > 0 for a real image, di < 0 for a virtual one, and m < 0 for an inverted image.

Critical angle at the cladding

sin θc = 1.42/1.5 = 0.9467 → θc = 71.2°

Numerical aperture

NA = √(1.5² − 1.42²) = 0.4833

Answer

NA = 0.4833

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